-
First Globular Cluster discovered.
The first globular cluster discovered, but then taken for a nebula, was M22 in Sagittarius, which was probably discovered by Abraham Ihle in 1665. -
Omega Centauri discovered
Southern Omega Centauri (NGC 5139) by Edmond Halley on his 1677 journey to St. Helena. -
M13 in Hercules
M13 in Hercules, again by Halley, in 1714 -
M15 and M2
Jean-Dominique Maraldi discovered M15 and M2 in September (1746) -
NGC 6712
Guillaume Legentil possibly or probably discovered NGC 6712 in 1749 -
M54
M54 found by Charles Messier -
M79
It was discovered by Pierre Méchain in 1780. M79 is at a distance of about 41,000 light years away from Earth and 60,000 light years away from the Galactic Center. -
M80 Discovered
M80 was discovered on January 4, 1781, by Charles Messier, who wrote, “The nebula is round, the center brilliant, and it resembles the nucleus of a little comet, surrounded with nebulosity.” William Herschel observed M80 four years later and called it “one of the richest and most compressed clusters of small stars I remember to have seen.” -
NGC 6553
NGC 6553 has yield range equal to old halo clusters. -
Dark Globular Clusters around Galaxy
Observations with ESO’s Very Large Telescope in Chile have discovered a new class of “dark” globular star clusters around this galaxy. These are marked in red. Normal globulars are marked in blue and globulars showing similar properties to dwarf galaxies are in green.